SDO HMI 2014-04-29 12:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.49 | 149.64 | 19.33 | 112.66 | -23.35 | 114.32 | 46.67 | 242.45 | 0.7553 | 412.4 | 236.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.90 | -23.59 | 115.90 | 48.24 | 242.69 | 0.7717 | -127.0 | -107.2 | |
| 25.49 | 134.40 | 19.33 | 101.87 | -23.36 | 114.75 | 47.10 | 242.62 | 0.7596 | 984.5 | 313.6 | |
| 0.00 | 1.96 | 0.00 | 1.41 | -18.53 | 112.83 | 45.17 | 248.39 | 0.7256 | -387.0 | -290.2 | |
| 0.00 | 0.98 | 0.00 | 0.75 | -25.24 | 114.84 | 47.19 | 240.27 | 0.7663 | 525.0 | 470.0 | |
| 0.00 | 1.25 | 0.00 | 0.90 | -21.16 | 112.59 | 44.94 | 244.78 | 0.7304 | -496.0 | -426.1 | |
| 0.00 | 1.34 | 0.00 | 0.96 | -21.22 | 112.11 | 44.46 | 244.55 | 0.7254 | -409.0 | -381.1 | |
| 0.00 | 1.96 | 0.00 | 1.40 | -21.40 | 111.64 | 43.98 | 244.14 | 0.7208 | -653.0 | -474.3 | |
| 0.00 | 1.60 | 0.00 | 1.13 | -22.86 | 110.58 | 42.92 | 241.80 | 0.7144 | -546.0 | -508.6 | |
| 0.00 | 1.16 | 0.00 | 0.81 | -22.50 | 110.04 | 42.38 | 242.07 | 0.7072 | -623.0 | -527.6 | |
| 0.00 | 0.45 | 0.00 | 0.31 | -25.29 | 107.90 | 40.25 | 237.38 | 0.6959 | -578.0 | -591.8 | |
| 0.00 | 0.62 | 0.00 | 0.43 | -25.94 | 107.99 | 40.34 | 236.56 | 0.6999 | -489.0 | -409.6 | |
| 0.00 | 1.34 | 0.00 | 0.89 | -27.58 | 104.27 | 36.62 | 232.34 | 0.6701 | -605.0 | -447.6 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -30.38 | 97.59 | 29.94 | 223.86 | 0.6235 | -673.0 | -540.1 | |
| 0.00 | 0.53 | 0.00 | 0.34 | -30.55 | 97.61 | 29.95 | 223.66 | 0.6250 | -638.0 | -511.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |